Environmental Engineering Reference
In-Depth Information
R i ε i B i Tð ð
1
k i W sec
θÞþk i sec
θWB i TðÞ
(19.48)
The Planck function can be expanded into a Taylor series about the brightness
temperature T i
in the form of
DB
DT T i
BT i ðÞ
DB
DT T i
DB
DT T j LTðÞ
R i ¼ B i TðÞ¼
j
¼
j
DB
DT T i T s T
DB
DT T i
B i TðÞB i TðÞþ
j
ð
Þ
¼
j
ð
T s T i þLTðÞ
Þ
DB
DT T i T a T i
DB
DT T i
B i TðÞB i TðÞþ
j
ð
Þ
¼
j
ð
T a T i þLTðÞ
Þ
ð
19
:
49
Þ
Inserting Eq. 19.49 into Eq. 19.48 will linearize the RTE with respect to
temperature:
LTðÞε i 1
ð
k i w sec
θ
Þ T s T i þLTðÞ
ð
Þ þ k i w sec
θ T a T i þLTðÞ
ð
Þ
(19.50)
Several approximations have been proposed for L ( T i ). Sun and Pinker ( 2003 )
use
LTðÞT i =n i
(19.51)
By inserting Eq. 19.51 into Eq. 19.50 ,
ð
C i 1 T i ε i T s
Þ ¼ T a ε i T s C i 2 T i
ð
Þ k i W sec
θ
(19.52a)
where
1
þ n i
ð
1
Þε i
ð
n i
1
Þ
ð
1
ε i
Þ
C i 1 ¼
; C i 2 ¼
(19.52b)
n i
n i
Let i represent the 11.0-
μ
m channel. For most land surfaces and the ocean, the
emissivity at 11.0
m is essentially unity.
In order to reduce the number of unknown variables, we assume that the
atmospheric mean temperature T a is proportional to the surface temperature T s :
μ
T a a w T s
(19.53)
It needs to be stated that assumption ( 19.53 ) may introduce errors if the surface
emissivity at 11.0-
μ
m channel is not close to unity. A solution for T s can be obtained
as follows:
T i
T 11
cW sec
T s
¼
(19.54)
½
ð
a w
1
Þk i W sec
θ þ
1
θ þ
1
Search WWH ::




Custom Search